Fig. 8.
Dependence of rtr/rcor from the magnetic field strength in the case of RZ Psc. The dotted line indicates the border between the magnetospheric accretion (below) and magnetic propeller (above) regimes. The unlabeled curve was computed assuming a mass accretion rate of 10−9 M⊙ yr−1 and illustrates pure magnetospheric accretion.
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